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1.1.6. Degenerating toric Calabi-Yau hypersurfaces [03YI]

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1.1.6. Degenerating toric Calabi-Yau hypersurfaces

A familiar picture from Riemann surface theory is that higher genus algebraic curves can be obtained topologically by patching together ‘pairs of pants’ along cylindrical necks. There is a similar picture for Calabi-Yau toric hypersurfaces approaching a large complex structure limit, well studied in tropical geometry. The discussions below are loosely based on Zharkov [32][31], and are included to predict the holomorphic structure of the positive and the negative vertices.

Let ℙ△\mathbb{P}_{\triangle} be a toric manifold whose moment polytope is the reflexive integral polytope △\triangle in ℝ4\mathbb{R}^{4}, so the integral points v∈△v\in\triangle correspond to a basis {sv}\{s_{v}\} for anticanonical sections. Let λ\lambda be a (suitably generic) function on △∩ℤ4\triangle\cap\mathbb{Z}^{4} whose piecewise linear extension is a convex function on ℝ4\mathbb{R}^{4} minimized at 0∈△0\in\triangle with minimum value 0. We consider a polarised family of hypersurfaces XtX_{t} defined by

(1.4) s0+∑v∈△∖{0}tλ⁡(v)​av​sv=0,s_{0}+\sum_{v\in\triangle\setminus\{0\}}t^{\lambda(v)}a_{v}s_{v}=0,

where ava_{v} are fixed nonzero complex numbers and tt is a small positive parameter. The holomorphic volume form is determined from the adjunction formula.

The key point is that when tt is very small, the hypersurface XtX_{t} decompose into a finite number of regions, on each of which only a small number of monomial functions svs0\frac{s_{v}}{s_{0}} dominate the rest. Thus up to scaling coordinates by powers of tt, there are only a small number of complex geometric local models, typically with some torus symmetry. Furthermore there is some combinatorial structure which controls how these local models patch together to give XtX_{t} as a complex manifold.

Example 1.1.

(Generic region) Suppose in some region only s0s_{0} and tλ⁡(v)​av​svt^{\lambda(v)}a_{v}s_{v} dominate, so the hypersurface locally looks like svs0=const\frac{s_{v}}{s_{0}}=\text{const}. After normalising by powers of tt we may write this as {z0=1}\{z_{0}=1\} in the coordinates z0,z1,z2,z3z_{0},z_{1},z_{2},z_{3} on the algebraic torus (ℂ∗)4(\mathbb{C}^{*})^{4}. This model has T3T^{3}-symmetry under the diagonal action on z1,z2,z3z_{1},z_{2},z_{3}. The T3T^{3}-orbits are the natural candidate for approximate SYZ fibres. Thus we naturally look for a Kähler metric with potential ϕ=ϕ⁡(u1,u2,u3)\phi=\phi(u_{1},u_{2},u_{3}) depending only on the logarithms u1=log⁡|z1|,u2=log⁡|z2|,u3=log⁡|z3|u_{1}=\log|z_{1}|,u_{2}=\log|z_{2}|,u_{3}=\log|z_{3}|. The holomorphic volume form Ω\Omega on the hypersurface is up to a scale factor given by

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡(z0−1)∧Ω,\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d(z_{0}-1)\wedge\Omega,

namely Ω=d​z1z1∧d​z2z2∧d​z3z3=d​log⁡z1∧d​log⁡z2∧d​log⁡z3\Omega=\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}. The complex Monge-Ampère equation (−1​∂∂¯​ϕ)3=const​−1​Ω∧Ω¯(\sqrt{-1}\partial\bar{\partial}\phi)^{3}=\text{const}\sqrt{-1}\Omega\wedge\overline{\Omega} naturally reduces to the real Monge-Ampère equation det(∂2ϕ∂ui​∂uj)=const\det(\frac{\partial^{2}\phi}{\partial u_{i}\partial u_{j}})=\text{const}. One can further calculate that such regions take up most of the volume measure on XtX_{t}, thus lending some evidence for the SYZ conjecture. We remark that the description only applies to local regions so the metrics are not complete.

Example 1.2.

The real Monge-Ampère equation governs also the region near the intersection of XtX_{t} with a smooth component of the toric boundary. Suppose after normalising by powers of tt, the dominant monomials are z0−1,z0−1​z1,z0−1​z2,z0−1​z3,1z_{0}^{-1},z_{0}^{-1}z_{1},z_{0}^{-1}z_{2},z_{0}^{-1}z_{3},1 in the coordinates z0,z1,z2,z3z_{0},z_{1},z_{2},z_{3} on the algebraic torus (ℂ∗)4(\mathbb{C}^{*})^{4}, so the hypersurface has the local complex geometric model {z0−1(1+z1+z2+z3)+1=0}⊂(ℂ∗)4\{z_{0}^{-1}(1+z_{1}+z_{2}+z_{3})+1=0\}\subset(\mathbb{C}^{*})^{4}, or equivalently −z0=1+z1+z2+z3-z_{0}=1+z_{1}+z_{2}+z_{3}. The adjunction formula

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡(z0−1​(1+z1+z2+z3)+1)∧Ω\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d(z_{0}^{-1}(1+z_{1}+z_{2}+z_{3})+1)\wedge\Omega

leads to Ω=d​z1z1∧d​z2z2∧d​z3z3\Omega=\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}} as before. The diagonal T3T^{3}-action on z1,z2,z3z_{1},z_{2},z_{3} provides the candidate for an approximate SYZ fibration, and a solution to the real Monge-Ampère equation in the log⁡|z1|,log⁡|z2|,log⁡|z3|\log|z_{1}|,\log|z_{2}|,\log|z_{3}| coordinates induces a local Calabi-Yau metric.

Example 1.3.

Suppose after normalising by powers of tt, the dominant monomials are (z1​z2)−1,−(z1​z2)−1​z3,−1(z_{1}z_{2})^{-1},-(z_{1}z_{2})^{-1}z_{3},-1, so the hypersurface admits the local complex geometric model {(z1z2)−1(1−z3)=1}⊂(ℂ∗)z0,z1,z2,z34\{(z_{1}z_{2})^{-1}(1-z_{3})=1\}\subset(\mathbb{C}^{*})^{4}_{z_{0},z_{1},z_{2},z_{3}}, or equivalently z1​z2=1−z3z_{1}z_{2}=1-z_{3}. This happens near the intersection of two smooth components of the toric boundary. Up to numerical factors, the holomorphic volume form is given by

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡((z1​z2)−1​(1−z3)−1)∧Ω,\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d((z_{1}z_{2})^{-1}(1-z_{3})-1)\wedge\Omega,

namely Ω=d​log⁡z0∧d​z1∧d​z2z3\Omega=d\log z_{0}\wedge\frac{dz_{1}\wedge dz_{2}}{z_{3}}. This model has a natural T2T^{2}-symmetry: one S1S^{1} acts trivially on z1,z2,z3z_{1},z_{2},z_{3} and rotates z0z_{0}, while the other S1S^{1} acts trivially on z0,z3z_{0},z_{3} and diagonally on z1,z2z_{1},z_{2}. The model is intimately related to the Ooguri-Vafa metric (cf. Section 1.3.2), and we expect this region to coincide with the neighbourhood of edges in the Gross-Ruan-Joyce picture.

In this paper we are primarily interested in the positive and negative vertices. These are relevant for certain regions near the intersection of XtX_{t} with some higher depth strata of the toric boundary of ℙ△\mathbb{P}_{\triangle}.

Example 1.4.

The positive vertex M+M^{+} describes a neighbourhood of the point (0,0,0,1)(0,0,0,1) inside {z0z1z2=1−z3}⊂ℂ3×ℂz3∗\{z_{0}z_{1}z_{2}=1-z_{3}\}\subset\mathbb{C}^{3}\times\mathbb{C}^{*}_{z_{3}}. In the toric hypersurface picture, we are looking at a region where the dominating monomials are up to scale factors (z0​z1​z2)−1,−z3​(z0​z1​z2)−1,1(z_{0}z_{1}z_{2})^{-1},-z_{3}(z_{0}z_{1}z_{2})^{-1},1, so the defining equation of XtX_{t} is approximately (z0​z1​z2)−1​(1−z3)=1(z_{0}z_{1}z_{2})^{-1}(1-z_{3})=1 once we absorb the scale factors into ziz_{i}. The holomorphic volume form Ω\Omega is up to constant given by

−−12​π​d​log​z0∧d​log​z1∧d​log​z2∧d​log​z3=d⁡((z0​z1​z2)−1​(1−z3)−1)∧Ω,-\frac{\sqrt{-1}}{2\pi}d\log z_{0}\wedge d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}=d((z_{0}z_{1}z_{2})^{-1}(1-z_{3})-1)\wedge\Omega,

or equivalently Ω=−−12​π​1z3​d​z0∧d​z1∧d​z2\Omega=-\frac{\sqrt{-1}}{2\pi}\frac{1}{z_{3}}dz_{0}\wedge dz_{1}\wedge dz_{2}. An important feature of this model is the diagonal T2T^{2}-symmetry:

ei​θ1⋅(z0,z1,z2)=(e−i​θ1​z0,ei​θ1​z1,z2),ei​θ2⋅(z0,z1,z2)=(e−i​θ2​z0,z1,ei​θ2​z2).e^{i\theta_{1}}\cdot(z_{0},z_{1},z_{2})=(e^{-i\theta_{1}}z_{0},e^{i\theta_{1}}z_{1},z_{2}),\quad e^{i\theta_{2}}\cdot(z_{0},z_{1},z_{2})=(e^{-i\theta_{2}}z_{0},z_{1},e^{i\theta_{2}}z_{2}).

We have Ω(∂∂θ1,∂∂θ2,⋅)=−−12​πdlogz3=dη\Omega(\frac{\partial}{\partial\theta_{1}},\frac{\partial}{\partial\theta_{2}},\cdot)=-\frac{\sqrt{-1}}{2\pi}d\log z_{3}=d\eta, where η=−−12​π​log⁡(z3)\eta=-\frac{\sqrt{-1}}{2\pi}\log(z_{3}) is a holomorphic coordinate with period 1, and takes the value zero at z0=z1=z2=0z_{0}=z_{1}=z_{2}=0. The relation between this complex geometric perspective and the topological picture in Section 1.1.3 is perhaps clearest with the generalised Gibbons-Hawking construction in mind (cf. Section 1.2 below). Essentially M+M^{+} is a singular T2T^{2}-bundle over a 4-dimensional base contained in ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta}, where μ1,μ2\mu_{1},\mu_{2} are the T2T^{2}-moment maps normalised to have value 0 at z0=z1=z2=0z_{0}=z_{1}=z_{2}=0. We shall notice that the discriminant locus 𝔇×{0}\mathfrak{D}\times\{0\} of this singular T2T^{2}-bundle is not sensitive to the choice of the Kähler form (cf. Lemma 1.6 and its ensuing Remark). The normalising constant on Ω\Omega imply that the SYZ T3T^{3}-fibres have ∫T3Ω=4​π2\int_{T^{3}}\Omega=4\pi^{2}.

Example 1.5.

The negative vertex M−M^{-} describes an open subset inside {z3z4=1−z1−z2}⊂ℂz1∗×ℂz2∗×ℂz3,z42\{z_{3}z_{4}=1-z_{1}-z_{2}\}\subset\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}\times\mathbb{C}^{2}_{z_{3},z_{4}}. In the toric hypersurface picture, we are looking at a region where the dominating monomials are up to scale factors just (z3​z4)−1(z_{3}z_{4})^{-1}, z1​(z3​z4)−1z_{1}(z_{3}z_{4})^{-1}, z2​(z3​z4)−1z_{2}(z_{3}z_{4})^{-1} and 1, so the defining equation of XtX_{t} is approximately (1−z1−z2)​(z3​z4)−1−1=0(1-z_{1}-z_{2})(z_{3}z_{4})^{-1}-1=0 once we absorb the scale factors into ziz_{i}. The holomorphic volume form Ω\Omega is given up to constant by

−14​π2​d​log​z1∧d​log​z2∧d​log​z3∧d​log​z4=d⁡((1−z1−z2)​(z3​z4)−1−1)∧Ω,\frac{\sqrt{-1}}{4\pi^{2}}d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}\wedge d\log z_{4}=d\left((1-z_{1}-z_{2})(z_{3}z_{4})^{-1}-1\right)\wedge\Omega,

or equivalently Ω=−−14​π2​1z1​z2​d​z2∧d​z3∧d​z4.\Omega=\frac{-\sqrt{-1}}{4\pi^{2}}\frac{1}{z_{1}z_{2}}dz_{2}\wedge dz_{3}\wedge dz_{4}. This model has S1S^{1}-symmetry:

ei​θ⋅(z1,z2,z3,z4)=(z1,z2,ei​θ​z3,e−i​θ​z4).e^{i\theta}\cdot(z_{1},z_{2},z_{3},z_{4})=(z_{1},z_{2},e^{i\theta}z_{3},e^{-i\theta}z_{4}).

Hence M−M^{-} is a singular S1S^{1}-bundle over ℝμ×ℂz1∗×ℂz2∗\mathbb{R}_{\mu}\times\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}, where μ\mu is the S1S^{1}-moment coordinate which takes the value zero on the singular locus {z3=z4=0}\{z_{3}=z_{4}=0\} (notice that the degeneracy of the S1S^{1} factor implies that the moment map is constant on this singular locus for any choice of Kähler form). This agrees with the modified topological description in Section 1.1.5. We calculate

ι∂∂θ​Ω=−14​π2​d​log⁡z1∧d​log⁡z2=d​η1∧d​η2,\iota_{\frac{\partial}{\partial\theta}}\Omega=-\frac{1}{4\pi^{2}}d\log z_{1}\wedge d\log z_{2}=d\eta_{1}\wedge d\eta_{2},

where the logarithmic coordinates ηp=12​π​−1​log⁡zp\eta_{p}=\frac{1}{2\pi\sqrt{-1}}\log z_{p} for p=1,2p=1,2 have period 1. The arg⁡z1,arg⁡z2\arg z_{1},\arg z_{2} coordinates provide a family of 2-tori in ℝ×ℂz1∗×ℂz2∗\mathbb{R}\times\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}, and the restriction of the S1S^{1}-bundle over these 2-tori defines a family of 3-tori. The normalising constant on Ω\Omega imply that ∫T3Ω=2​π\int_{T^{3}}\Omega=2\pi.

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